Comparison of continuous star formation models with the observed SED. The data are corrected for extinction equivalent to E(B − V) = 0.3. The four solid lines represent (from bottom to top): 5, 10, 50, and 500 Myr models. The dashed line is a combination the 10 Myr model (15% by mass) and a 1 Gyr single‐burst model (85% by mass). The models are scaled to match the optical data (1200–3000 Å rest).